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  MESA meets MURaM. Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations

Ball, W. H., Beeck, B., Cameron, R. H., & Gizon, L. (2016). MESA meets MURaM. Surface effects in main-sequence solar-like oscillators computed using three-dimensional radiation hydrodynamics simulations. Astronomy and Astrophysics, 592: A159. doi:10.1051/0004-6361/201628300.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-002B-5FE6-5 Version Permalink: http://hdl.handle.net/21.11116/0000-0007-24D2-3
Genre: Journal Article

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 Creators:
Ball, W. H.1, Author              
Beeck, B.2, Author              
Cameron, R. H.1, 3, Author              
Gizon, L.1, Author              
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              
2IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
3Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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 MPIS_GROUPS: Solar and Stellar Interiors
 MPIS_PROJECTS: SFBA18
 Abstract: -

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 Dates: 2016
 Publication Status: Published in print
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361/201628300
BibTex Citekey: Ball:2016-075
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Publ. Info: -
Pages: - Volume / Issue: 592 Sequence Number: A159 Start / End Page: - Identifier: -